A relativistic outflow model: Analytical solutions

Details A relativistic outflow model: Analytical solutions A relativistic outflow model: Analytical solutions

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..555s&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

1

Galactic Nuclei, Circumnuclear Matter, And Bulges, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

Calculations of highly energetic neutrino and TeV γ-ray emission from relativistic jets of active galactic nuclei (AGN) are often based on numerically derived solutions. We present analytical solutions for a relativistic collision front model that allow to perform parameter studies. The solutions are used to study distributions of energetic protons as well as a tool to compare γ-ray spectra originating from the decay of neutral pions to observational results e.g. from Blazars.

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